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The Direction of Ejection of Photo-electrons Produced by X-rays

D. H. Loughridge

  • Norman Bridge Laboratory, California Institute of Technology, Pasadena, California

Phys. Rev. 26, 697 – Published 1 December, 1925

DOI: https://doi.org/10.1103/PhysRev.26.697

Abstract

Stereoscopic photographs of photo-electrons produced by 40 kv Mo Kα x-rays, were examined by a stereoscopic comparator which gave a quantitative measure of the initial direction of ejection in space. The measurement of twenty-four distinct tracks in a series of twenty-nine pairs of photographs showed that the most probable angle of ejection was about 70° with the primary beam. This supports the view that the electric vector of the radiation plays a very important part in the production of photo-electrons. The small forward or backward component, noticed in many tracks, must come from the random momentum of the electron in its orbit before ejection.

References (5)

  1. Bothe, Zeits. f. Phys. 26, 59-73 (1924)
  2. P. Auger, Comptes Rendus 178, 929 (1924)
  3. C. T. R. Wilson, Proc. Roy. Soc. 104, p. 1 (1923)
  4. Bubb, Phys. Rev. 23, p. 137 (1924)
  5. Bubb, Phil. Mag. 49, p. 824 (1925)

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